The high spatial resolution of the Chandra and upgraded Giant Metrewave Radio Telescope (GMRT) allow us to study the interplay between X-ray-emitting hot gas and nonthermal radio emission.
We have obtained new upgraded GMRT data, and have used archive GMRT and Chandra data of the nearby \(z\)  = 0.0726 [1]} richness class 2 cluster, A2065, which is one of the 10 galaxy clusters that make up the Corona Borealis supercluster.
[2]} noted that two cD galaxies dominate the cluster center in the optical and their radial velocities differ by \(\sim \) 600 km s\(^{-1}\) .
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